A possible indication of the insufficiency of the simplistic homogeneous models to estimate the magnetic fields of the CME using the emission of turosincrotron by Devojyoti Kansabanik et al. – European astronomer radio community
Coronal mass ejections (CME) are expulsions of plasma and large -scale magnetic field of the solar crown to the Helosphere. The magnetic field dragged into the CME plasma is crucial to understand its propagation, evolution and geo -ffectivity. Among the different observables in the radio wavelengths, the spectral modeling of the IMINCROTRON DIRECTRÓN (GS) emission…